Powering luminous core collapse supernovae with jets

Abstract

I examine recent fittings of luminous supernovae (LSNe) with extra energy sources of magnetar and helium burning and find that in about half of these LSNe the fitting parameters have some problems. In some LSNe the total energy of these two energy sources is larger than the kinetic energy of the ejecta that the fitting yields. In some others LSNe the total energy of the delayed neutrino explosion mechanism and these two extra sources combined is smaller than the kinetic energy that the fitting yields. These difficulties suggest that, like earlier claims that jets power superluminous supernovae (SLSNe), jets also power the less luminous LSNe. A magnetar might also supply energy. However, in most cases jets supply more energy than the magnetar, during the explosion and possibly at late times. I strengthen an earlier claim that jets launched at magnetar birth cannot be ignored. I explain the trend of maximum rise time for a given luminosity of hydrogen deficient core collapse supernovae (CCSNe), in particular LSNe and SLSNe, with a toy model of jets that are active for a long time after explosion.

arXiv commentAccepted for publication in The Astrophysical Journal

References in corpus (58)

• How Massive Single Stars End their Life
• Explosion Mechanisms of Core-Collapse Supernovae
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
• Supernovae, Jets, and Collapsars
• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Core-Collapse Supernova Explosion Theory
• Jet-Induced Explosions of Core Collapse Supernovae
• Relativistic Jets from Collapsars
• A very luminous magnetar-powered supernova associated with an ultra-long gamma-ray burst
• The magnetar model for Type I superluminous supernovae I: Bayesian analysis of the full multicolour light curve sample with MOSFiT
• The Diversity of Transients from Magnetar Birth
• Relativistic MHD simulations of core-collapse GRB jets: 3D instabilities and magnetic dissipation
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
• Revival of The Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor Star
• The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_{\odot }$ Stars
• The intermediate r-process in core-collapse supernovae driven by the magneto-rotational instability
• The jet feedback mechanism (jfm) in stars, galaxies and clusters
• Three-dimensional AMR simulations of long-duration Gamma-Ray Burst jets inside massive progenitor stars
• Black Hole Accretion Discs and Luminous Transients in Failed Supernovae from Non-Rotating Supergiants
• The Type Icn SN 2021csp: Implications for the Origins of the Fastest Supernovae and the Fates of Wolf-Rayet Stars
• The Hydrodynamic Origin of Neutron Star Kicks
• Explaining the most energetic supernovae with an inefficient jet-feedback mechanism
• A statistical study of super-luminous supernovae in the magnetar engine model and implications for their connection with gamma-ray bursts and hypernovae
• Triggering jet-driven explosions of core-collapse supernovae by accretion from convective regions
• Results from a systematic survey of X-ray emission from Hydrogen-poor Superluminous Supernovae
• Magnetar-powered superluminous supernovae must first be exploded by jets
• A Common Central Engine for Long Gamma Ray Bursts and Type Ib/c Supernovae?
• The Most Luminous Supernovae
• Core collapse supernova remnants with ears
• Three-dimensional simulation of a core-collapse supernova for a binary star progenitor of SN 1987A
• A Planar Jitternig-Jets Pattern in Core-Collapse Supernova Explosions
• A call for a paradigm shift from neutrino-driven to jet-driven core-collapse supernova mechanisms
• Angular momentum fluctuations in the convective helium shell of massive stars
• Applying the Jet Feedback Mechanism to Core-Collapse Supernova Explosions
• The imprints of the last jets in core collapse supernovae
• The chemical signature of jet-driven hypernovae
• Implications of turbulence for jets in core-collapse supernova explosions
• Jets launched at magnetar birth cannot be ignored
• Observability of inflated companion stars after supernovae in massive binaries
• Four (Super)luminous Supernovae from the First Months of the ZTF Survey
• Supplying angular momentum to the jittering jets explosion mechanism using inner convection layers
• Nothing to see here: Failed supernovae are faint or rare
• Reviving the stalled shock by jittering jets in core collapse supernovae: jets from the standing accretion shock instability
• Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae
• The Energy Sources of Superluminous Supernovae
• Ultra-delayed neutrino-driven explosion of rotating massive-star collapse
• The two promising scenarios to explode core collapse supernovae
• Imprints of the jittering jets explosion mechanism in the morphology of the supernova remnant SNR 0540-69.3
• Emission peaks in the light curve of core collapse supernovae by late jets
• Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
• The magnetar model of the superluminous supernova GAIA16apd and the explosion jet feedback mechanism (JFM)
• Amplifying magnetic fields of a newly born neutron star by stochastic angular momentum accretion in core collapse supernovae
• Numerically investigating the peculiar periphery of a supernova remnant in the medium with a density gradient: the case of RCW 103
• Jet-shaped geometrically modified light curves of core collapse supernovae
• An explanation for the peculiar periphery of supernova remnant G309.2-0.6
• Explosion Energies for Core-collapse Supernovae I: Analytic, Spherically Symmetric Solutions

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• The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
• A population of Type Ibc supernovae with massive progenitors; broad lightcurves not uncommon in (i)PTF
• Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
• The $\gamma$-process nucleosynthesis in core-collapse supernovae II. Effect of the explosive recipe
• Feeding post core collapse supernova explosion jets with an inflated main sequence companion
• Pre-explosion, explosion, and post-explosion jets in supernova SN 2019zrk
• Rapid decline in the lightcurves of luminous supernovae by jet-driven bipolar explosions